nearby galaxy evolution prof. gerhardt r meurer. galaxy evolution in a nutshell galaxy evolution2 ...
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Nearby Galaxy Evolution
Prof. Gerhardt R Meurer
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Galaxy Evolution 2
Galaxy evolution in a nutshell
Time machinesThe farther we peerThe farther back in time we see
Reveal cosmic historyHubble: to < 1 Gyr after big
bangWMAP, Planck: to < 1 Myr
The nearby universeSee recent evolutionSee galaxies in exquisite detailCan detect the faintest galaxiesGalaxies stabilizing
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Galaxy Evolution 3
Transformation
The Star Formation Cycle Interstellar gas clouds
cool and collapse Stars form (also planets...) Stars expel gas
o stellar windso supernovae explosions
Some of the material returns to a gas phaseo hottero brightero enriched
• hot gas• heavy elements• energy• radiation
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Galaxy Evolution 4
We can see this happen
Examples NGC3603: young star cluster NGC1705: exploding galaxy
Many telescopes needed cool gas: radio young stars: optical, UV Explosions, hot gas: optical,
X-ray
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Galaxy Evolution 5
Surveying star formation
An international effort Parkes 64m: cool hydrogen CTIO1.5m: hot hydrogen GALEX: hottest stars (UV)
All types of gas-rich galaxies Big spirals little dwarfs Interactions / mergers Unexpected companions
Science What types of stars form? Where do stars form? How is SF regulated? What is total cosmic SF rate?
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Galaxy Evolution 6
Other Facilities I Use (or will use) Hubble Space Telescope Pan-STARRS1 1.8m SkyMapper 1.3m Australian National University
2.3m WIYN 3.5m Australia Telescope Compact
Array Wide-field Infrared Survey
Explorer (WISE) Australia Square Kilometre
Array Pathfinder (ASKAP)
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Galaxy Evolution 77
My Collaborations with the USA
Johns Hopkins University (Baltimore, MD) Space Telescope Science Institute (Baltimore, MD) National Science Foundation (Washington DC) Carnegie Observatories (Pasadena CA) U. California, Santa Cruz Arizona State University (Phoenix AZ) University of Massachusetts (HST proposal) University of Colorado (NASA Small Mission Explorer proposal)
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Galaxy Evolution 88
Larger collaborations Murchison Wide Field Array
Three US Partner institutions MOU PanSTARRS1 & ICRAR
Analyze the light of thousands of galaxies Large Synoptic Survey Telescope
See Wicenec presentation Square Kilometre Array
Many interested scientist in the USA